摘要

Continuous-flow spin-exchange optical pumping (SEOP) continues to serve as the most widespread method of polarizing Xe-129 for magnetic resonance experiments. Unfortunately, continuous-flow SEOP still suffers from as-yet unidentified inefficiencies that prevent the production of large volumes of xenon with a nuclear spin polarization close to theoretically calculated values. In this work we use a combination of ultra-low field nuclear magnetic resonance spectroscopy and atomic absorption spectroscopy (AAS) measurements to study the effects of dark Rb vapor on hyperpolarized Xe-129 in situ during continuous-flow SEOP. We find that dark Rb vapor in the optical cell outlet has negligible impact on the final Xe-129 polarization at typical experimental conditions, but can become significant at higher oven temperatures and lower flow rates. Additionally, in the AAS spectra we also look for a signature of paramagnetic Rb clusters, previously identified as a source of xenon depolarization and a cause for SEOP inefficiency, for which we are able to set an upper limit of 8.3 x 10(15) Rb dimers per cm(3).

  • 出版日期2017-6